{"paper":{"title":"Loop Quantum Gravity Effects on the High Energy Cosmic Ray Spectrum","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Center for Mathematical Sciences, Gonzalo A. Palma (Department of Applied Mathematics, Jorge Alfaro (Facultad de F\\'isica, Pontificia Universidad Cat\\'olica de Chile), Theoretical Physics, University of Cambridge)","submitted_at":"2005-01-14T21:05:21Z","abstract_excerpt":"Recent observations on ultra high energy cosmic rays (those cosmic rays with energies greater than $\\sim 4 \\times 10^{18}$ eV) suggest an abundant flux of incoming particles with energies above $1 \\times 10^{20}$ eV. These observations violate the Greisen-Zatsepin-Kuzmin cutoff. To explain this anomaly we argue that quantum-gravitational effects may be playing a decisive role in the propagation of ultra high energy cosmic rays. We consider the loop quantum gravity approach and provide useful techniques to establish and analyze constraints on the loop quantum gravity parameters arising from obs"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/0501116","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}